The results are reported of a search that was carried out in September
1993 for slow moving objects in the Solar System that may be potentia
l members of the Kuiper belt of comets. Two objects, 1993 SB and 1993
SC were discovered and an analysis of all the images allows a possible
rotation rate for 1993 SC to be determined. An estimate, based on the
limiting magnitudes of the images, is made of the likely space densit
y of such objects. (C) 1995 Academic Press, Inc.